Superstring theory and integration over the moduli space

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1 Superstring theory and integration over the moduli space Kantaro Ohmori Hongo,The University of Tokyo Oct, 23rd, 2013 arxiv: [KO,Yuji Tachikawa] Todai/Riken joint workshop on Super Yang-Mills, solvable systems and related subjects

2 Section 1 introduction

3 Simplified history of the superstring theory

4 Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize

5 Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize 84 :1st superstring revolution

6 Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize 84 :1st superstring revolution 86: Conformal Invariance, Supersymmetry, and String Theory [D.Friedan, E.Martinec, S.Shenker]

7 Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize 84 :1st superstring revolution 86: Conformal Invariance, Supersymmetry, and String Theory [D.Friedan, E.Martinec, S.Shenker] 94 :2nd superstring revolution ) nonperturbative perspective

8 Simplified history of the superstring theory 70 s:bosonic string theory! supersymmetrize 84 :1st superstring revolution 86: Conformal Invariance, Supersymmetry, and String Theory [D.Friedan, E.Martinec, S.Shenker] 94 :2nd superstring revolution ) nonperturbative perspective 12: Superstring Perturbation Theory Revisited [E.Witten]: Superstring perturbation theory and supergeometry

9 Bosonic string theory

10 Bosonic string theory Action:S = R d2 zg j

11 Bosonic string theory Action:S = R d2 zg j ) Riemann Surface = 2d surface + metric

12 Bosonic string theory Action:S = R d2 zg j ) Riemann Surface = 2d surface + metric Conformal symmetry ) bc ghost

13 Bosonic string theory Action:S = R d2 zg j ) Riemann Surface = 2d surface + metric Conformal symmetry ) bc ghost )A= R M bos,g dmd mf (m, m)

14 Superstring theory

15 Superstring theory Action:S = R d2 zd 2 G ij D X i D X j

16 Superstring theory Action:S = R d2 zd 2 G ij D X i D X j ) Super Riemann Surface =2dsurface+supermetric =2dsurface+metric + gravitino θ θ θ θ θ θ θ θ θ

17 Superstring theory Action:S = R d2 zd 2 G ij D X i D X j ) Super Riemann Surface =2dsurface+supermetric =2dsurface+metric + gravitino θ θ θ θ θ θ θ θ θ Superconformal symmetry ) BC(bc ) superghost

18 Superstring theory Action:S = R d2 zd 2 G ij D X i D X j ) Super Riemann Surface =2dsurface+supermetric =2dsurface+metric + gravitino θ θ θ θ θ θ θ θ θ Superconformal symmetry ) BC(bc ) superghost )A= R M super,g dmd d md F (m, m,, )

19 Superstring theory Action:S = R d2 zd 2 G ij D X i D X j ) Super Riemann Surface =2dsurface+supermetric =2dsurface+metric + gravitino θ θ θ θ θ θ θ θ θ Superconformal symmetry ) BC(bc ) superghost )A= R M super,g dmd d md F (m, m,, )? )A= R M spin,g dmd mf 0 (m, m)

20 The bosonic and super moduli space M super 6=M spin odd direction M super M spin

21 The bosonic and super moduli space M super 6=M spin odd direction M super M spin Global integration on M super 6) Global integration on M spin (preserving holomorphic factorization)

22 The work of [KO,Tachikawa]

23 The work of [KO,Tachikawa] Global integration on M super 6) Global integration on M spin

24 The work of [KO,Tachikawa] Global integration on M super 6) Global integration on M spin We found special cases where Global integration on M super ) Global integration on M spin

25 The work of [KO,Tachikawa] (2)

26 The work of [KO,Tachikawa] (2) 2concreteexamples

27 The work of [KO,Tachikawa] (2) 2concreteexamples N =0 N =1embedding [N. Berkovits,C. Vafa 94]

28 The work of [KO,Tachikawa] (2) 2concreteexamples N =0 N =1embedding [N. Berkovits,C. Vafa 94] Topological amplitudes [I. Antoniadis, E. Gava, K.S. Narain, T.R. Taylor 94] [M. Bershadsky, S. Cecotti, H. Ooguri, C. Vafa 94]

29 1 introduction 2 Supergeometry and Superstring 3 Reduction to integration over bosonic moduli

30 Supermanifold

31 Supermanifold supermanifold = patched superspaces

32 Supermanifold supermanifold = patched superspaces M :supermanifoldofdimensionp q M 3 (x 1,, x p 1,, q ) i j = j i

33 Supermanifold supermanifold = patched superspaces M :supermanifoldofdimensionp q M 3 (x 1,, x p 1,, q ) i j = j i x 0 i = f i (x ) 0 µ = µ(x ) U α

34 Supermanifold supermanifold = patched superspaces M :supermanifoldofdimensionp q M 3 (x 1,, x p 1,, q ) i j = j i x 0 i = f i (x ) 0 µ = µ(x ) M red = {(x i,, x p )},! M U α

35 Supermoduli space Msuper

36 Supermoduli space M super Space of deformations of SRS (Super Riemann Surface)

37 Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red )

38 Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red ) odd deformation: z 2 H 1 ( red, T 1/2 red )

39 Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red ) odd deformation: z 2 H 1 ( red, T 1/2 red ) { }: basisofgravitinob.g) =

40 Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red ) odd deformation: z 2 H 1 ( red, T 1/2 red ) { }: basisofgravitinob.g) = dim M super = e o =3g 3 2g 2 (g 2)

41 Supermoduli space M super Space of deformations of SRS (Super Riemann Surface) even deformation: µ z z 2 H 1 ( red, T red ) odd deformation: z 2 H 1 ( red, T 1/2 red ) { }: basisofgravitinob.g) = dim M super = e o =3g 3 2g 2 (g 2) M super,red 'M spin

42 Supermoduli space of SRS with punctures

43 Supermoduli space of SRS with punctures n NS NS punctures and n R Rpunctures

44 Supermoduli space of SRS with punctures n NS NS punctures and n R Rpunctures dim M super = e o =3g 3+n NS +n R 2g 2+n NS +n R /2 (g 2)

45 Coupling between gravitino and SCFT

46 Coupling between gravitino and SCFT S = 1 R 2 d 2 z T F

47 Coupling between gravitino and SCFT S = 1 R 2 d 2 z T F S e = 1 R 2 d 2 z e TF e

48 Coupling between gravitino and SCFT S = 1 R 2 d 2 z T F S e = 1 R 2 d 2 z e TF e S e = R d 2 z ea A / µ e µ (Flat background)

49 Coupling between gravitino and SCFT S = 1 R 2 d 2 z T F S e = 1 R 2 d 2 z e TF e S e = R d 2 z ea A / µ e µ (Flat background) c.f. D µ D µ 3 A µ A µ

50 Scattering amplitudes of superstring

51 Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R)

52 Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R) A V,g = R M super dmd d md F V,g (m,, m, )

53 Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R) A V,g = R M super dmd d md F V,g (m,, m, ) FD V,g (m,, m, ) = Q i V Q e i a=1 (R red d 2 zbµ a ) Q e b=1 (R red d 2 zb e eµ b ) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) exp( S S e S e )i m

54 Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R) A V,g = R M super dmd d md F V,g (m,, m, ) FD V,g (m,, m, ) = Q i V Q e i a=1 (R red d 2 zbµ a ) Q e b=1 (R red d 2 zb e eµ b ) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) exp( S S e S e )i m S = P R o =1 2 red d 2 z T F

55 Scattering amplitudes of superstring V i :Vertexop.pic.number 1 (NS) or 1/2 (R) A V,g = R M super dmd d md F V,g (m,, m, ) FD V,g (m,, m, ) = Q i V Q e i a=1 (R red d 2 zbµ a ) Q e b=1 (R red d 2 zb e eµ b ) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) exp( S S e S e )i m S = P R o =1 2 red d 2 z T F We get result of FMS when = (z p ) and int. out. s.

56 Integration over a supermanifold

57 Integration over a supermanifold E = {(m 1, 2 )}/ m m m +1

58 Integration over a supermanifold E = {(m 1, 2 )}/ m m m +1 R E (a + b 1 2 )dmdmd 1 d 2 = b= + p 1a/2

59 Integration over a supermanifold E = {(m 1, 2 )}/ m m m +1 R E (a + b 1 2 )dmdmd 1 d 2 = b= + p 1a/2 1 2 mixed with m

60 Projectedness of supermanifolds

61 Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed

62 Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed, p : M! M red exists

63 Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed, p : M! M red exists R M! = R M red p (!)

64 Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed, p : M! M red exists R M! = R M red p (!) All supermanifolds are projected in smooth sense.

65 Projectedness of supermanifolds M:projected, an atlas in which x 0 = f (x) for all gluing ) naive integrations with s are allowed, p : M! M red exists R M! = R M red p (!) All supermanifolds are projected in smooth sense. Complex supermanifolds are not projected in holomorphic sense in general.

66 Supermoduli Space is not projected [R.Donagi, E.Witten, arxiv: ]

67 Supermoduli Space is not projected [R.Donagi, E.Witten, arxiv: ] M super,red 'M spin i : M spin,! M super

68 Supermoduli Space is not projected [R.Donagi, E.Witten, arxiv: ] M super,red 'M spin i : M spin,! M super p : M super!m spin does not exists. (g 5, non-holomorphiconeexists)

69 Supermoduli Space is not projected [R.Donagi, E.Witten, arxiv: ] M super,red 'M spin i : M spin,! M super p : M super!m spin does not exists. (g 5, non-holomorphiconeexists) Global integration on M super 6) Global integration on M spin (preserving holomorphic factorization)

70 Section 3 Reduction to integration over bosonic moduli

71 Reduction condition

72 Reduction condition Global integration on M super ) Global integration on M spin in special cases F (m, m,, ) =G(m, m) Q all i i (saturations of s)

73 Reduction condition Global integration on M super ) Global integration on M spin in special cases F (m, m,, ) =G(m, m) Q all i i (saturations of s) mixing of m and (m 0 = m )doesnot changes F

74 Reduction condition Global integration on M super ) Global integration on M spin in special cases F (m, m,, ) =G(m, m) Q all i i (saturations of s) mixing of m and (m 0 = m )doesnot changes F F does not depend on the locations of picture changing operators

75 Topological amplitudes in string theory [I. Antoniadis, E. Gava, K.S. Narain, T.R. Taylor 94] [M. Bershadsky, S. Cecotti, H. Ooguri, C. Vafa 94]

76 Topological amplitudes in string theory [I. Antoniadis, E. Gava, K.S. Narain, T.R. Taylor 94] [M. Bershadsky, S. Cecotti, H. Ooguri, C. Vafa 94] Type II string on CY (N =(2, 2)SCFT) R 1,3 ) 4d N =2supergravity model

77 Topological amplitudes in string theory [I. Antoniadis, E. Gava, K.S. Narain, T.R. Taylor 94] [M. Bershadsky, S. Cecotti, H. Ooguri, C. Vafa 94] Type II string on CY (N =(2, 2)SCFT) R 1,3 ) 4d N =2supergravity model F-term of 4d e ective field theory is related to topological string.

78 Reduction to topological string Type II string on CY(6d) R 1,3 ) 4d N =2supergravity model

79 Reduction to topological string Type II string on CY(6d) R 1,3 ) 4d N =2supergravity model A g :zeromomentalimitofg loop amplitude of 2g 2 graviphotons (RR) and 2 gravitons (NSNS)

80 Reduction to topological string Type II string on CY(6d) R 1,3 ) 4d N =2supergravity model A g :zeromomentalimitofg loop amplitude of 2g 2 graviphotons (RR) and 2 gravitons (NSNS) A g = R M super

81 Reduction to topological string Type II string on CY(6d) R 1,3 ) 4d N =2supergravity model A g :zeromomentalimitofg loop amplitude of 2g 2 graviphotons (RR) and 2 gravitons (NSNS) A g = R M super A g =(g!) 2 F g = R M bos

82 Vertex operators

83 Vertex operators Graviphoton: V T = spacetime (ghost) p = exp(i 3 2 (H(z) H(z))) e H : U(1) R boson : U(1) R charge (3/2, 3/2)

84 Vertex operators Graviphoton: V T = spacetime (ghost) p = exp(i 3 2 (H(z) H(z))) e H : U(1) R boson : U(1) R charge (3/2, 3/2) Graviton: V R = R red spacetime,ghost

85 Saturation of s

86 Saturation of s A g = R D Q 2g 2 i =1 (x i ) U(1) R :(3g 3, 3g 3) (spacetime) (bc) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) R exp( red (T F + T e E F e + A e )) m

87 Saturation of s A g = R D Q 2g 2 i =1 (x i ) U(1) R :(3g 3, 3g 3) (spacetime) (bc) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) R exp( red (T F + T e E F e + A e )) m nonzero contribution ) 3g 3 and 3g 3e

88 Saturation of s A g = R D Q 2g 2 i =1 (x i ) U(1) R :(3g 3, 3g 3) (spacetime) (bc) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) R exp( red (T F + T e E F e + A e )) m nonzero contribution ) 3g 3 and 3g 3e There are only 3g 3 and 3g 3 e

89 Saturation of s A g = R D Q 2g 2 i =1 (x i ) U(1) R :(3g 3, 3g 3) (spacetime) (bc) Q o=1 ( R d2 red z ) Q e o =1 ( R red d 2 z e e ) R exp( red (T F + T e E F e + A e )) m nonzero contribution ) 3g 3 and 3g 3e There are only 3g 3 and 3g 3 e The correlation function does not depend of the choice of

90 Conclusion

91 Conclusion Superstring amplitude cannot be represent as integration over M spin in general

92 Conclusion Superstring amplitude cannot be represent as integration over M spin in general Special cases exist.

93 Conclusion Superstring amplitude cannot be represent as integration over M spin in general Special cases exist. Amplitudes which is equivalent topological amplitudes are the case.

94 End.

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